106272018-10-10Computational Modeling of Ablative Materials: Application to Phenolic PyrolysisCompletedAug 2011Jan 2012<p>Many NASA missions (ESMD, SMD), including crewed missions to Mars, are not possible with current ablative materials. Improved understanding will (1) facilitate the design of new, novel ablative materials and (2) improve material response models used for TSP design. We will demonstrate and validate phenolic pyrolysis simulation methods using reactive potentials (REAX), Density Functional Tight Binding (DFTB) and Density Functional Theory (DFT).<p/><p>Ablative materials are required for the most demanding atmospheric reentry missions. These materials are often carbon fibers embedded in a phenolic polymer matrix. At high temperature, phenolic undergoes pyrolysis where the polymer is transformed into a pure carbon solid called char. Pyrolysis is an endothermic, chemically reactive process, and is the only in-depth energy absorbing mechanism used in ablative systems. High char yield is desirable to minimize mass loss into gaseous products. Importantly, polymer char yields can vary substantially. Further, thermal and mechanical properties of the pyrolyzed material can be very different from the original material. Optimizing properties of the char surface layer is crucial, since it is the part of the TSP in direct contact with the hot reentry plasma. A robust pyrolysis simulation methodology (which does not currently exist) will aid in understanding the structure and properties of phenolic and in developing new polymers with higher char yield and char with improved properties. In addition, more accurate material response models, used to design TSP, will result, thereby leading to reduced safety margins, and thus reduced mass/cost of the TPS. We will perform atomistic pyrolysis simulations using REAX, DFTB and DFT to demonstrate the different methods, and in particular to validate REAX for pyrolysis of realistic polymers (phenolic and otherwise). In addition, we will obtain important insights into chemical kinetics of early stage pyrolysis. These same methods can also be applied to other reactive processes (oxidation, sublimation, etc) and other problems in ablative materials modeling (polymer properties, interfaces, materials design, etc). This project resulted in the following journal publications: "Comparison of REAXFF, DFTB and DFT for Phenolic Pyrolysis. 1. Molecular Dynamics Simulations", T. Qi, C.W. Bauschlicher, J.W. Lawson, T.G. Desai, E.J. Reed, J. Phys. Chem. A 117, (2013), p. 11115 "Comparison of REAXFF, DFTB and DFT for Phenolic Pyrolysis. 2. Elementary Reaction Paths", C.W. Bauschlicher, T. Qi, E.J. Reed, A. Lenfant, J.W. Lawson, T.G. Desai, J. Phys. Chem. A 117, (2013), p. 11126 </p><p><p>Many NASA missions (ESMD, SMD), including crewed missions to Mars, are not possible with current ablative materials. Computational modeling will enable the rapid and efficient development of the next generation of high performance ablators that are critical for NASA entry vehicles. We believe that this technology will enable ESMD and SMD missions.</p></p>11132479Entry, Descent, and Landing Systems33029.1Aeroassist and Atmospheric Entry324911Modeling, Simulation, Information Technology and Processing325012Materials, Structures, Mechanical Systems and ManufacturingCenter Innovation Fund: ARC CIFSpace Technology Mission DirectorateAmes Research CenterARCNASA CenterMoffett FieldCAAdvanced Cooling Technologies, Inc.IndustryLancasterPACaliforniaTherese GriebelJohn W LawsonJohn W Lawson87281676 Approval (# 17536)Story<p>Ames Approval dated 11/26/14</p>1563Comparison of ReaxFF, DFTB, and DFT for Phenolic Pyrolysis. 1. Molecular Dynamics SimulationsLinkhttp://pubs.acs.org/doi/abs/10.1021/jp40810961564Comparison of ReaxFF, DFTB, and DFT for Phenolic Pyrolysis. 2. Elementary Reaction PathsLinkhttp://pubs.acs.org/doi/abs/10.1021/jp408113w1565Graphical abstractImageCombination of molecular dynamics simulations and computational chemistry was used to study thermal decomposition of phenolic resins2963https://techport.nasa.gov/file/296344806